Journal: Monthly Notices of the Royal Astronomical Society

  • Publication
    The origin of the light distribution in spiral galaxies
    We analyse a high-resolution, fully cosmological, hydrodynamical disc galaxy simulation, to study the source of the double-exponential light profiles seen in...
  • Publication
    The origin of the mid-infrared nuclear polarization of active galactic nuclei
    We combine new (NGC 1275, NGC 4151, and NGC 5506) and previously published (Cygnus A, Mrk 231, and NGC 1068) sub-arcsecond resolution mid-infrared (MIR; 8-13 μm...
  • Publication
    The origin of the tilted disc in the low-mass X-ray binary GR Mus (XB 1254-690)
    We present photometric and spectroscopic observations of the low-mass X-ray binary GR Mus (XB 1254-690), and find strong evidence for the presence of a negative...
  • Publication
    The origins of post-starburst galaxies at z < 0.05
    Post-starburst galaxies can be identified via the presence of prominent Hydrogen Balmer absorption lines in their spectra. We present a comprehensive study of...
  • Publication
    The outburst radial velocity curve of X-ray Nova Scorpii 1994 (= GRO J1655-40): a reduced mass for the black hole?
    We present a re-analysis of the outburst radial velocity data for X-ray Nova Scorpii 1994. Using a model based on X-ray heating of the secondary star, we...
  • Publication
    The outbursting protostar 2MASS 22352345 + 7517076 and its environment
    We studied the Class I protostar 2MASS 22352345 + 7517076 whose dramatic brightening between the IRAS, Akari, and WISE surveys was reported by Onozato et al...
  • Publication
    The Padova-Millennium Galaxy and Group Catalogue (PM2GC): the group-finding method and the PM2GC catalogues of group, binary and single field galaxies
    We present the construction and describe the properties of the Padova-Millennium Galaxy and Group Catalogue (PM2GC), a galaxy catalogue representative of the...
  • Publication
    The PARSEC view of star formation in galaxy centres: from protoclusters to star clusters in an early-type spiral
    Understanding star formation in galaxies requires resolving the physical scale on which star formation often occurs: the scale of star clusters. We present a...
  • Publication
    The PAU survey: classifying low-z SEDs using Machine Learning clustering
    We present an application of unsupervised Machine Learning clustering to the PAU survey of galaxy spectral energy distribution (SED) within the COSMOS field...